55 Cancri d

Planet· orbits 55 Cancri

55 Cancri d - the outermost planet, a cold gas giant of about 4 Jupiter masses on a wide 13-year orbit, one of the first Jupiter-analogue exoplanets found. Its mass is measured; it has never transited, so its size is model-based.

Open in 3D viewSee 55 Cancri d in the live, interactive 3D map

Key facts

Mass
7.36 × 10²⁷ kg
3.88 M♃ (1,233 M⊕)
Year
13.1 Earth years
4,799 Earth days
Distance from 55 Cancri
5.6 AU

Science

Physical

Mass
7.36 × 10²⁷ kg · 3.88 M♃ (1,233 M⊕)
Radius
Not measured
No transit — radius is a model estimate for a ~4-Jupiter gas giant; no density is quoted.

Orbital

Semi-major axis
5.6 AU
From the NASA Exoplanet Archive (radial-velocity orbit)
Eccentricity
0.091
From the NASA Exoplanet Archive (radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (radial-velocity orbit)
Orbital period
13.14 years
From the NASA Exoplanet Archive (radial-velocity orbit)
Perihelion
5.09 AU
Computed from the orbital elements
Aphelion
6.11 AU
Computed from the orbital elements
Mean orbital velocity
12.7 km/s
Computed from the orbital elements

Composition

Bulk composition
A cold gas giant of true mass ~4 Jupiter — one of the first Jupiter-analogue exoplanets found (2002). Never imaged.
Cloud appearance
Appearance based on ESO/M. Kornmesser's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
0.0202 S⊕ · 2% of the sunlight Earth receives
Computed from 55 Cancri's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
105 K (-168 °C)
Computed model value for its cold 5.6-AU orbit — not measured.

Discovery & history

Method
Radial-velocity detection (stellar wobble)
Name
Designated 'd' under the IAU convention that letters a star's planets 'b', 'c', 'd'... in the order they are discovered (the star itself is the unwritten 'a').

Announced in 2002, it was among the first exoplanets found on a wide, Jupiter-like orbit around a Sun-like star.

Images

No official imagery available — this object has never been visited and no officially-licensed depiction exists.